J
J. A. Miralles
Researcher at University of Alicante
Publications - 22
Citations - 755
J. A. Miralles is an academic researcher from University of Alicante. The author has contributed to research in topics: Neutron star & Magnetic field. The author has an hindex of 9, co-authored 22 publications receiving 699 citations.
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Magneto-thermal evolution of neutron stars
TL;DR: In this article, the authors studied the mutual influence of thermal and magnetic evoluti on in a neutron star's crust in axial symmetry, and showed that the feedback between Joule heating and magnetic diffusion is strong, resulting in a faster dissipation of the stronger fields during the first 10 5 − 10 6 years of a star's life.
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Population synthesis studies of isolated neutron stars with magnetic field decay
TL;DR: In this article, population synthesis of different types of neutron stars (thermally emitting isolated NSs, normal radio pulsars, magnetars) was performed taking into account the magnetic field decay and using results from the most recent advances in NS cooling theory.
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Anisotropic thermal emission from magnetized neutron stars
TL;DR: In this article, the thermal emission from isolated neutron stars with strong magnetic fields B > 10 13 G was studied to explain the origin of the anisotropy in the surface temperature distribution.
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Thermal radiation from magnetic neutron star surfaces
TL;DR: In this paper, the authors investigated the thermal emission from magnetic neutron star surfaces in which the cohesive effects of the magnetic field have produced the condensation of the atmosphere and the external layers.
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Stability analysis of relativistic jets from collapsars and its implications on the short-term variability of gamma-ray bursts
TL;DR: In this paper, the transverse structure and stability properties of relativistic jets formed in the course of the collapse of a massive progenitor were investigated and the presence of a strong shear in the bulk velocity of such jets was shown to be responsible for a very rapid shear driven instability that arises for any velocity profile.